Table B.1
Summary of observations.
| Reference | Target | Observation | DIT (s) × NDIT × NCYCLE | Exposure | DIMM seeing | |
|---|---|---|---|---|---|---|
| number | name | date | time (min) | (′′) | ||
| 1 | WW Cha | 12-03-17 | 32 × 2 × 6 | 25.6 | 0.42−0.55 | |
| 2 | Sz 45 | 13-03-17 | 96 × 1 × 6 | 38.4 | 0.45−0.78 | |
| 3 | IK Lup | 07-03-17 | 96 × 1 × 4 | 25.6 | 0.36−0.50 | |
| 4 | HT Lup | 13-03-17 | 64 × 1 × 9 | 38.4 | 0.39−0.73 | |
| 5 | 2MASS J16035767-2 031 055 | 11-03-17 | 96 × 1 × 4 | 25.6 | 0.33−0.49 | |
| 6 | 2MASS J16062196-1 928 445 | 13-03-17 | 96 × 1 × 5 | 32.0 | 0.41−0.67 | |
| 7 | 2MASS J16064385-1 908 056 | 07-03-17 | 96 × 1 × 4 | 25.6 | 0.40−0.50 | |
| 8 | HK Lup | 11-03-17 | 96 × 1 × 6 | 38.4 | 0.34−0.46 | |
| 9 | V1094 Sco | 12-03-17 | 96 × 1 × 6 | 38.4 | 0.36−0.51 | |
| 10 | 2MASS J16090075-1 908 526 | 07-03-17 | 96 × 1 × 4 | 25.6 | 0.47−0.62 | |
| 11 | 2MASS J16102857-1 904 469 | 07-03-17 | 32 × 2 × 6 | 25.6 | 0.63−0.94 | |
| 12 | 2MASS J16111534-1 757 214 | 07-03-17 | 96 × 1 × 6 | 38.4 | 0.40−0.63 | |
| 13 | 2MASS J16141107-2 305 362 | 13-03-17 | 64 × 2 × 4 | 34.1 | 0.43−0.58 | |
| 14 | 2MASS J16142029-1 906 481 | 13-03-17 | 64 × 1 × 5 | 34.1 | 0.50−0.60 | |
| 96 × 1 × 2 | ||||||
| 15 | VV Sco | 12-03-17 | 64 × 1 × 8 | 34.1 | 0.45−0.54 | |
| 16 | 2MASS J16154416-1 921 171 | 12-03-17 | 96 × 1 × 6 | 38.4 | 0.44−0.58 | |
| 17 | DoAr 16 | 11-03-17 | 64 × 1 × 6 | 25.6 | 0.54−0.91 | |
| 18 | EM* SR4 | 12-03-17 | 32 × 2 × 8 | 34.1 | 0.40−0.55 | |
| 19 | DoAr 21 | 11-03-17 | 16 × 4 × 2 | 34.1 | 0.38−0.58 | |
| 32 × 2 × 6 | ||||||
| 20 | DoAr 25 | 07-03-17 | 96 × 1 × 6 | 38.4 | 0.50−0.67 | |
| 21 | EM* SR9 | 11-03-17 | 96 × 1 × 6 | 38.4 | 0.37−0.73 |
Notes. Columns are the reference number in this work, the target name, the observation date, the individual integration time (DIT) multiplied by the number of integrations (NDIT) and the number of polarimetric cycles (NCYCLES), the total integration time, and DIMM seeing during the observations. The total integration time is obtained from DIT (s) × NDIT × NCYCLE × 4 because each polarimetric cycle is composed of four Stokes setups (Q+, Q−, U+, and U−).
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